Nothing Special   »   [go: up one dir, main page]

CERN Accelerating science

Article
Report number arXiv:1502.01592
Title Planck 2015 results. XVII. Constraints on primordial non-Gaussianity
Author(s)

Ade, P.A.R. (Cardiff U.) ; Aghanim, N. (Orsay, IAS) ; Arnaud, M. (AIM, Saclay) ; Arroja, F. (INFN, Padua ; Taiwan, Natl. Taiwan U.) ; Ashdown, M. (Cambridge U., KICC ; Cambridge U.) ; Aumont, J. (Orsay, IAS) ; Baccigalupi, C. (INFN, Trieste ; SISSA, Trieste) ; Ballardini, M. (IASF, Bologna ; INFN, Bologna ; Bologna U.) ; Banday, A.J. (IRAP, Toulouse ; Toulouse III U.) ; Barreiro, R.B. (Cantabria U., Santander) ; Bartolo, N. (Padua U. ; INFN, Padua) ; Basak, S. (INFN, Trieste ; SISSA, Trieste) ; Battaner, E. (Granada U., Theor. Phys. Astrophys.) ; Benabed, K. (Paris, Inst. Astrophys.) ; Benoît, A. (Neel Lab, Grenoble) ; Benoit-Lévy, A. (University Coll. London ; Paris, Inst. Astrophys.) ; Bernard, J.P. (IRAP, Toulouse ; Toulouse III U.) ; Bersanelli, M. (Milan U. ; IASF, Milan) ; Bielewicz, P. (Warsaw, Copernicus Astron. Ctr. ; IRAP, Toulouse ; Toulouse III U. ; INFN, Trieste ; SISSA, Trieste) ; Bock, J.J. (Caltech, JPL ; Caltech) ; Bonaldi, A. (Manchester U.) ; Bonavera, L. (Cantabria U., Santander) ; Bond, J.R. (Canadian Inst. Theor. Astrophys.) ; Borrill, J. (Darmstadt, EMMI ; LBL, Berkeley ; UC, Berkeley, Space Sci. Dept.) ; Bouchet, F.R. (Paris, Inst. Astrophys.) ; Boulanger, F. (Orsay, IAS) ; Bucher, M. (APC, Paris) ; Burigana, C. (IASF, Bologna ; Ferrara U. ; INFN, Bologna) ; Butler, R.C. (IASF, Bologna) ; Calabrese, E. (Oxford U.) ; Cardoso, J.F. (APC, Paris ; Paris, Inst. Astrophys.) ; Catalano, A. (LPSC, Grenoble ; Paris Observ.) ; Challinor, A. (Cambridge U., Inst. of Astron. ; Cambridge U., KICC ; Cambridge U., DAMTP) ; Chamballu, A. (AIM, Saclay ; IRFU, SPP, Saclay ; Orsay, IAS) ; Chiang, H.C. (Princeton U. ; KwaZulu Natal U.) ; Christensen, P.R. (Bohr Inst.) ; Church, S. (Stanford U., Phys. Dept.) ; Clements, D.L. (Imperial Coll., London) ; Colombi, S. (Paris, Inst. Astrophys.) ; Colombo, L.P.L. (Southern California U. ; Caltech, JPL) ; Combet, C. (LPSC, Grenoble) ; Couchot, F. (Orsay, LAL) ; Coulais, A. (Paris Observ.) ; Crill, B.P. (Caltech, JPL ; Caltech) ; Curto, A. (Cantabria U., Santander ; Cambridge U. ; Cambridge U., KICC) ; Cuttaia, F. (IASF, Bologna) ; Danese, L. (INFN, Trieste ; SISSA, Trieste) ; Davies, R.D. (Manchester U.) ; Davis, R.J. (Manchester U.) ; de Bernardis, P. (Rome U.) ; De Rosa, A. (IASF, Bologna) ; De Zotti, G. (Padua Observ. ; INFN, Trieste ; SISSA, Trieste) ; Delabrouille, J. (APC, Paris) ; Désert, F.X. (IPAG) ; Diego, J.M. (Cantabria U., Santander) ; Dole, H. (Orsay, IAS ; IUF, Paris) ; Donzelli, S. (IASF, Milan) ; Doré, O. (Caltech, JPL ; Caltech) ; Douspis, M. (Orsay, IAS) ; Ducout, A. (Paris, Inst. Astrophys. ; Imperial Coll., London) ; Dupac, X. (ESA, Madrid) ; Efstathiou, G. (Cambridge U., Inst. of Astron.) ; Elsner, F. (University Coll. London ; Paris, Inst. Astrophys.) ; Enßlin, T.A. (Garching, Max Planck Inst., MPE) ; Eriksen, H.K. (Inst. Theor. Astrophys., Oslo) ; Fergusson, J. (Cambridge U., DAMTP) ; Finelli, F. (IASF, Bologna ; INFN, Bologna) ; Forni, O. (IRAP, Toulouse ; Toulouse III U.) ; Frailis, M. (Trieste Observ.) ; Fraisse, A.A. (Princeton U.) ; Franceschi, E. (IASF, Bologna) ; Frejsel, A. (Bohr Inst.) ; Galeotta, S. (Trieste Observ.) ; Galli, S. (Chicago U., KICP) ; Ganga, K. (APC, Paris) ; Gauthier, C. (APC, Paris ; Taiwan, Natl. Taiwan U.) ; Ghosh, T. (Orsay, IAS) ; Giard, M. (IRAP, Toulouse ; Toulouse III U.) ; Giraud-Héraud, Y. (APC, Paris) ; Gjerløw, E. (Inst. Theor. Astrophys., Oslo) ; González-Nuevo, J. (Oviedo U. ; Cantabria U., Santander) ; Górski, K.M. (Caltech, JPL ; Warsaw U. Observ.) ; Gratton, S. (Cambridge U., KICC ; Cambridge U., Inst. of Astron.) ; Gregorio, A. (Trieste U. ; Trieste Observ. ; INFN, Trieste) ; Gruppuso, A. (IASF, Bologna) ; Gudmundsson, J.E. (Stockholm U., OKC ; Nordita ; Princeton U.) ; Hamann, J. (CERN ; Sydney U.) ; Hansen, F.K. (Inst. Theor. Astrophys., Oslo) ; Hanson, D. (McGill U. ; Caltech, JPL ; Canadian Inst. Theor. Astrophys.) ; Harrison, D.L. (Cambridge U., Inst. of Astron. ; Cambridge U., KICC) ; Heavens, A. (Imperial Coll., London) ; Helou, G. (Caltech) ; Henrot-Versillé, S. (Orsay, LAL) ; Hernández-Monteagudo, C. (CEFCA, Teruel ; Garching, Max Planck Inst., MPE) ; Herranz, D. (Cantabria U., Santander) ; Hildebrandt, S.R. (Caltech, JPL ; Caltech) ; Hivon, E. (Paris, Inst. Astrophys.) ; Hobson, M. (Cambridge U.) ; Holmes, W.A. (Caltech, JPL) ; Hornstrup, A. (Denmark, Tech. U.) ; Hovest, W. (Garching, Max Planck Inst., MPE) ; Huang, Z. (Canadian Inst. Theor. Astrophys.) ; Huffenberger, K.M. (Florida State U.) ; Hurier, G. (Orsay, IAS) ; Jaffe, A.H. (Imperial Coll., London) ; Jaffe, T.R. (IRAP, Toulouse ; Toulouse III U.) ; Jones, W.C. (Princeton U.) ; Juvela, M. (Helsinki Inst. of Phys. ; Helsinki U.) ; Keihänen, E. (Helsinki Inst. of Phys. ; Helsinki U.) ; Keskitalo, R. (Darmstadt, EMMI ; LBL, Berkeley) ; Kim, J. (Garching, Max Planck Inst., MPE) ; Kisner, T.S. (LBL, Berkeley) ; Knoche, J. (Garching, Max Planck Inst., MPE) ; Kunz, M. (Geneva U., Dept. Theor. Phys. ; Orsay, IAS ; African Inst. Math. Sci., Cape Town) ; Kurki-Suonio, H. (Helsinki U. ; Helsinki Inst. of Phys.) ; Lacasa, F. (Orsay, IAS ; Sao Paulo, IFT) ; Lagache, G. (Marseille, Lab. Astrophys. ; Orsay, IAS) ; Lähteenmäki, A. (Aalto U. ; Helsinki Inst. of Phys.) ; Lamarre, J.M. (Paris Observ.) ; Lasenby, A. (Cambridge U. ; Cambridge U., KICC) ; Lattanzi, M. (Ferrara U.) ; Lawrence, C.R. (Caltech, JPL) ; Leonardi, R. (Brasilia U.) ; Lesgourgues, J. (Aachen, Tech. Hochsch. ; CERN) ; Levrier, F. (Paris Observ.) ; Lewis, A. (Sussex U.) ; Liguori, M. (Padua U. ; INFN, Padua) ; Lilje, P.B. (Inst. Theor. Astrophys., Oslo) ; Linden-Vørnle, M. (Denmark, Tech. U.) ; López-Caniego, M. (ESA, Madrid ; Cantabria U., Santander) ; Lubin, P.M. (UC, Santa Barbara) ; Macías-Pérez, J.F. (LPSC, Grenoble) ; Maggio, G. (Trieste Observ.) ; Maino, D. (Milan U. ; IASF, Milan) ; Mandolesi, N. (IASF, Bologna ; Ferrara U.) ; Mangilli, A. (Orsay, IAS ; Orsay, LAL) ; Marinucci, D. (Rome U., Tor Vergata) ; Maris, M. (Trieste Observ.) ; Martin, P.G. (Canadian Inst. Theor. Astrophys.) ; Martínez-González, E. (Cantabria U., Santander) ; Masi, S. (Rome U.) ; Matarrese, S. (Padua U. ; INFN, Padua ; GSSI, Aquila) ; McGehee, P. (Caltech, IPAC) ; Meinhold, P.R. (UC, Santa Barbara) ; Melchiorri, A. (Rome U. ; INFN, Rome) ; Mendes, L. (ESA, Madrid) ; Mennella, A. (Milan U. ; IASF, Milan) ; Migliaccio, M. (Cambridge U., Inst. of Astron. ; Cambridge U., KICC) ; Mitra, S. (IUCAA, Pune ; Caltech, JPL) ; Miville-Deschênes, M.A. (Orsay, IAS ; Canadian Inst. Theor. Astrophys.) ; Moneti, A. (Paris, Inst. Astrophys.) ; Montier, L. (IRAP, Toulouse ; Toulouse III U.) ; Morgante, G. (IASF, Bologna) ; Mortlock, D. (Imperial Coll., London) ; Moss, A. (Nottingham U.) ; Münchmeyer, M. (Paris, Inst. Astrophys.) ; Munshi, D. (Cardiff U.) ; Murphy, J.A. (NUIM, Maynooth) ; Naselsky, P. (Bohr Inst.) ; Nati, F. (Princeton U.) ; Natoli, P. (Ferrara U. ; ASDC, Frascati ; IASF, Bologna) ; Netterfield, C.B. (Toronto U., Astron. Dept.) ; Nørgaard-Nielsen, H.U. (Denmark, Tech. U.) ; Noviello, F. (Manchester U.) ; Novikov, D. (IMCS, Moscow) ; Novikov, I. (Bohr Inst. ; IMCS, Moscow) ; Oxborrow, C.A. (Denmark, Tech. U.) ; Paci, F. (INFN, Trieste ; SISSA, Trieste) ; Pagano, L. (Rome U. ; INFN, Rome) ; Pajot, F. (Orsay, IAS) ; Paoletti, D. (IASF, Bologna ; INFN, Bologna) ; Pasian, F. (Trieste Observ.) ; Patanchon, G. (APC, Paris) ; Peiris, H.V. (University Coll. London) ; Perdereau, O. (Orsay, LAL) ; Perotto, L. (LPSC, Grenoble) ; Perrotta, F. (INFN, Trieste ; SISSA, Trieste) ; Pettorino, V. (U. Heidelberg, ITP) ; Piacentini, F. (Rome U.) ; Piat, M. (APC, Paris) ; Pierpaoli, E. (Southern California U.) ; Pietrobon, D. (Caltech, JPL) ; Plaszczynski, S. (Orsay, LAL) ; Pointecouteau, E. (IRAP, Toulouse ; Toulouse III U.) ; Polenta, G. (ASDC, Frascati ; Rome Observ.) ; Popa, L. (Bucharest, Inst. Space Science) ; Pratt, G.W. (AIM, Saclay) ; Prézeau, G. (Caltech ; Caltech, JPL) ; Prunet, S. (Paris, Inst. Astrophys.) ; Puget, J.L. (Orsay, IAS) ; Rachen, J.P. (Nijmegen U., IMAPP ; Garching, Max Planck Inst., MPE) ; Racine, B. (APC, Paris) ; Rebolo, R. (IAC, La Laguna ; CSIC, Madrid ; Laguna U., Tenerife) ; Reinecke, M. (Garching, Max Planck Inst., MPE) ; Remazeilles, M. (Manchester U. ; Orsay, IAS ; APC, Paris) ; Renault, C. (LPSC, Grenoble) ; Renzi, A. (Rome U., Tor Vergata ; INFN, Rome) ; Ristorcelli, I. (IRAP, Toulouse ; Toulouse III U.) ; Rocha, G. (Caltech, JPL ; Caltech) ; Rosset, C. (APC, Paris) ; Rossetti, M. (Milan U. ; IASF, Milan) ; Roudier, G. (APC, Paris ; Paris Observ. ; Caltech, JPL) ; Rubiño-Martín, J.A. (IAC, La Laguna ; Laguna U., Tenerife) ; Rusholme, B. (Caltech, IPAC) ; Sandri, M. (IASF, Bologna) ; Santos, D. (LPSC, Grenoble) ; Savelainen, M. (Helsinki U. ; Helsinki Inst. of Phys.) ; Savini, G. (University Coll. London) ; Scott, D. (British Columbia U.) ; Seiffert, M.D. (Caltech, JPL ; Caltech) ; Shellard, E.P.S. (Cambridge U., DAMTP) ; Shiraishi, M. (Padua U. ; INFN, Padua) ; Smith, K. (Perimeter Inst. Theor. Phys.) ; Spencer, L.D. (Cardiff U.) ; Stolyarov, V. (Cambridge U. ; Stavropol, Astrophys. Observ. ; Kazan State U.) ; Stompor, R. (APC, Paris) ; Sudiwala, R. (Cardiff U.) ; Sunyaev, R. (Garching, Max Planck Inst., MPE ; Moscow, Space Res. Inst.) ; Sutter, P. (Paris, Inst. Astrophys.) ; Sutton, D. (Cambridge U., Inst. of Astron. ; Cambridge U., KICC) ; Suur-Uski, A.S. (Helsinki U. ; Helsinki Inst. of Phys.) ; Sygnet, J.F. (Paris, Inst. Astrophys.) ; Tauber, J.A. (ESTEC, Noordwijk) ; Terenzi, L. (Florence U. ; IASF, Bologna) ; Toffolatti, L. (Oviedo U. ; Cantabria U., Santander ; IASF, Bologna) ; Tomasi, M. (Milan U. ; IASF, Milan) ; Tristram, M. (Orsay, LAL) ; Troja, A. (Milan U.) ; Tucci, M. (Geneva U., Dept. Theor. Phys.) ; Tuovinen, J. (Trinity Coll., Dublin) ; Valenziano, L. (IASF, Bologna) ; Valiviita, J. (Helsinki U. ; Helsinki Inst. of Phys.) ; van Tent, B. (Orsay, LPT) ; Vielva, P. (Cantabria U., Santander) ; Villa, F. (IASF, Bologna) ; Wade, L.A. (Caltech, JPL) ; Wandelt, B.D. (Paris, Inst. Astrophys. ; Illinois U., Urbana (main)) ; Wehus, I.K. (Caltech, JPL ; Inst. Theor. Astrophys., Oslo) ; Yvon, D. (IRFU, SPP, Saclay) ; Zacchei, A. (Trieste Observ.) ; Zonca, A. (UC, Santa Barbara)

Publication 2016-09-20
Imprint 05 Feb 2015
Number of pages 66
Note Comments: 61 pages, 27 figures, 31 tables. This paper is one of a set associated with the 2015 data release from Planck
68 pages, 32 figures, 31 tables. Subsection 6.3 on "Primordial curvature reconstruction" added; analysis in subsection 8.3 extended (paragraph "High frequency resonance model estimator" added); introduction to Section 10 and Appendix B added. This paper is one of a set associated with the 2015 data release from Planck. Matches version accepted for publication in Astronomy & Astrophysics
In: Astron. Astrophys. 594 (2016) A17
DOI 10.1051/0004-6361/201525836
Subject category Astrophysics and Astronomy
Abstract The Planck full mission cosmic microwave background(CMB) temperature and E-mode polarization maps are analysed to obtain constraints on primordial non-Gaussianity(NG). Using three classes of optimal bispectrum estimators - separable template-fitting (KSW), binned, and modal - we obtain consistent values for the local, equilateral, and orthogonal bispectrum amplitudes, quoting as our final result from temperature alone fNL^local=2.5+\-5.7, fNL^equil=-16+\-70 and fNL^ortho=-34+\-33(68%CL). Combining temperature and polarization data we obtain fNL^local=0.8+\-5.0, fNL^equil=-4+\-43 and fNL^ortho=-26+\-21 (68%CL). The results are based on cross-validation of these estimators on simulations, are stable across component separation techniques, pass an extensive suite of tests, and are consistent with Minkowski functionals based measurements. The effect of time-domain de-glitching systematics on the bispectrum is negligible. In spite of these test outcomes we conservatively label the results including polarization data as preliminary, due to a known mismatch of the noise model in simulations and the data. Beyond fNL estimates, we present model-independent reconstructions of the CMB bispectrum and derive constraints on early universe scenarios that generate NG, including general single-field and axion inflation, initial state modifications, parity-violating tensor bispectra, and directionally-dependent vector models. We also present a wide survey of scale-dependent oscillatory bispectra, and we look for isocurvature NG. Our constraint on the local primordial trispectrum amplitude is gNL^local=(-9.0+\-7.7)x10^4 (68%CL), and we perform an analysis of additional trispectrum shapes. The global picture is one of consistency with the premises of the LambdaCDM cosmology, namely that the structure we observe today was sourced by adiabatic, passive, Gaussian, and primordial seed perturbations.[abridged]
Copyright/License arXiv nonexclusive-distrib. 1.0



Corresponding record in: Inspire


 Registro creado el 2015-02-06, última modificación el 2024-05-03


Texto completo:
Descargar el texto completoPDF
Enlace externo:
Descargar el texto completoPreprint